Renyi Type Holographic Dark Energy
| dc.contributor.author | Aktaş, Arzu | |
| dc.contributor.author | Yılmaz, İhsan | |
| dc.date.accessioned | 2025-01-27T19:37:16Z | |
| dc.date.available | 2025-01-27T19:37:16Z | |
| dc.date.issued | 2024 | |
| dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
| dc.description.abstract | Dark energy is one of the prominent mysteries of the universe that still awaits a solution. One of the plausible ways to collect data about any formation or understand its information capacity is to investigate the entropy of that formation. In this study, Renyi Holographic Dark Energy (RHDE) matter distribution is analyzed within the framework of General Relativity Theory, considering homogeneous and isotropic Friedmann-Robertson- Walker (FRW) space-time. Hubble parameter and RHDE density were used to obtain exact solutions of Einstein field equations. The analysis of the obtained solutions was performed by drawing evolution graphs for redshift z. | |
| dc.identifier.doi | 10.53570/jnt.1509610 | |
| dc.identifier.endpage | 47 | |
| dc.identifier.issn | 2149-1402 | |
| dc.identifier.issue | 48 | |
| dc.identifier.startpage | 40 | |
| dc.identifier.trdizinid | 1270636 | |
| dc.identifier.uri | https://doi.org/10.53570/jnt.1509610 | |
| dc.identifier.uri | https://search.trdizin.gov.tr/tr/yayin/detay/1270636 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.12428/17173 | |
| dc.indekslendigikaynak | TR-Dizin | |
| dc.language.iso | en | |
| dc.relation.ispartof | Journal of New Theory | |
| dc.relation.publicationcategory | Makale - Ulusal Hakemli Dergi - Kurum Öğretim Elemanı | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.snmz | KA_TRD_20250125 | |
| dc.subject | Hubble parameter | |
| dc.subject | Renyi holographic dark energy | |
| dc.subject | FRW universe model | |
| dc.title | Renyi Type Holographic Dark Energy | |
| dc.type | Article |
